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herschel [2018/10/09 15:10]
Déborah Paradis
herschel [2021/01/27 10:12]
Déborah Paradis
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 The photometric bands are centered at 70, 100 and 160 microns for PACS, and at 250, 350 and 500 microns for SPIRE, with an angular resolution going from 5 arcsec to 37 arcsec. The photometric bands are centered at 70, 100 and 160 microns for PACS, and at 250, 350 and 500 microns for SPIRE, with an angular resolution going from 5 arcsec to 37 arcsec.
  
-CADE currently only serves SPIRE photometric data for each Key-Programs. Healpix maps at 250 microns and 350 microns have been smoothed to 37 arcsec. ​+CADE currently only serves SPIRE photometric data for each Key-Programs. Healpix maps at 250 microns and 350 microns have been smoothed to 37 arcsec. We also provide Healpix maps at 4' angular resolution.
 The units of the Healpix maps are MJy/sr. The units of the Healpix maps are MJy/sr.
  
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 |[[Herschel Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\ ​ |[[Herschel Galactic Cold Cores|Galactic Cold Cores (PI: M. Juvela & I. Ristorcelli)]]|\\ ​
 |[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]| ​ \\ |[[Herschel GOODS|GOODS- The Great Observatories Origins Deep Survey: far-infrared imaging with Herschel (PI: D. Elbaz)]]| ​ \\
 +|[[Herschel Gould Belt|Gould Belt- Probing the origin of the stellar initial mass function: A wide-field Herschel photometric survey of nearby star-forming cloud complexes (PI: P. André)]]| ​ \\
 |[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\ |[[Herschel H-atlas|H-ATLAS- The Herschel Thousand Degree Survey (PI: S. Eales)]]|\\
 |[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\ |[[Herschel Lensing Survey|Herschel Lensing Survey (PI: E. Egami)]]|\\